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8/9/2019 Module P7 L2
http://slidepdf.com/reader/full/module-p7-l2 1/5
Module P7 Observing the
Universe
Lesson 2
8/9/2019 Module P7 L2
http://slidepdf.com/reader/full/module-p7-l2 2/5
Summer Sky, Winter Sky
Orion visible in
December
Orion not visible in
June
8/9/2019 Module P7 L2
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Reminder Positions on the Earth are measured
using latitude and longitude.
For example, London has a latitude
of 51º 32¶ N and a longitude of 0º 5¶W. (Longitude is along the equator)
(Note 5¶: = 5 minutes of arc = 5/60ths
of a degree)
See link for other cities
8/9/2019 Module P7 L2
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From Earth, the stars
appear to be bright dots
fixed to the inside of a
giant ball or sphere.
This sphere is
completely imaginar y,
but it is called ³the
Celestial Sphere´.
Celestial North Pole
Celestial South
Pole
Celestial Equator
Ecliptic ± path of
highest point of Sun
during a whole year
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Declination is the
celestial equivalent of
latitude. It gives you
the ³height´ in degreesabove the celestial
equator.
RA or right ascension
is the celestial
equivalent of longitude.It gives you the
³distance along´ the
celestial equator.
It would be sensible tomeasure it in degrees.
However , astronomers
measure it in hours
and minutes instead,
with 24 hours
equivalent to 360º.